DiRAC-3 Operations 2019-2022 - Cambridge [2020-06 resubmission]
Lead Research Organisation:
University of Cambridge
Department Name: Institute of Astronomy
Abstract
DiRAC-3 Operations 2019-2022 resubmission; This is an administrative resubmission to replace ST/S003800/1 which has already been peer-reviewed.
Organisations
Publications
Ježo T
(2023)
Resonance-aware NLOPS matching for off-shell $$ t\overline{t} $$ + tW production with semileptonic decays
in Journal of High Energy Physics
Pierens A
(2023)
Three-dimensional evolution of radiative circumbinary discs: The size and shape of the inner cavity
in Astronomy & Astrophysics
Daly RT
(2023)
Successful kinetic impact into an asteroid for planetary defence.
in Nature
Sherletov A
(2023)
Lattice Studies of 3D Maximally Supersymmetric Yang-Mills
Sergeev D
(2023)
Simulations of idealised 3D atmospheric flows on terrestrial planets using LFRic-Atmosphere
in Geoscientific Model Development
Trotta D
(2023)
Three-dimensional modelling of the shock-turbulence interaction
in Monthly Notices of the Royal Astronomical Society
Ho C
(2024)
Shallower radius valley around low-mass hosts: evidence for icy planets, collisions, or high-energy radiation scatter
in Monthly Notices of the Royal Astronomical Society
Dong-Páez C
(2024)
The Uchuu-SDSS galaxy light-cones: a clustering, redshift space distortion and baryonic acoustic oscillation study
in Monthly Notices of the Royal Astronomical Society
Mak M
(2024)
3D simulations of TRAPPIST-1e with varying CO2, CH4, and haze profiles
in Monthly Notices of the Royal Astronomical Society
Roth A
(2024)
Hot Jupiter diversity and the onset of TiO/VO revealed by a large grid of non-grey global circulation models
in Monthly Notices of the Royal Astronomical Society
Scharré L
(2024)
The effects of stellar and AGN feedback on the cosmic star formation history in the simba simulations
in Monthly Notices of the Royal Astronomical Society
He Q
(2024)
Unveiling lens light complexity with a novel multi-Gaussian expansion approach for strong gravitational lensing
in Monthly Notices of the Royal Astronomical Society
Schoettler C
(2024)
The effect of dynamical interactions in stellar birth environments on the orbits of young close-in planetary systems
in Monthly Notices of the Royal Astronomical Society
Dhandha J
(2024)
Decaying turbulence in molecular clouds: how does it affect filament networks and star formation?
in Monthly Notices of the Royal Astronomical Society
Thompson O
(2024)
Predictions for CO emission and the CO-to-H2 conversion factor in galaxy simulations with non-equilibrium chemistry
in Monthly Notices of the Royal Astronomical Society
Changeat Q
(2024)
Is the Atmosphere of the Ultra-hot Jupiter WASP-121 b Variable?
in The Astrophysical Journal Supplement Series
Dutta R
(2024)
Metal line emission around z < 1 galaxies
in Astronomy & Astrophysics
Bonino A
(2024)
Mapping eccentricity evolutions between numerical relativity and effective-one-body gravitational waveforms
in Physical Review D
Aslanyan V
(2024)
A New Field Line Tracer for the Study of Coronal Magnetic Topologies
in The Astrophysical Journal
Bennett E
(2024)
Mixing between flavor singlets in lattice gauge theories coupled to matter fields in multiple representations
in Physical Review D
Berné O
(2024)
A far-ultraviolet-driven photoevaporation flow observed in a protoplanetary disk
in Science
Elsender D
(2024)
An implicit algorithm for simulating the dynamics of small dust grains with smoothed particle hydrodynamics
in Monthly Notices of the Royal Astronomical Society
Kong (??) S
(2024)
Filamentary Molecular Cloud Formation via Collision-induced Magnetic Reconnection in a Cold Neutral Medium
in The Astrophysical Journal
Vijayan A
(2024)
First Light And Reionisation Epoch Simulations (FLARES) - XII: The consequences of star-dust geometry on galaxies in the EoR
in Monthly Notices of the Royal Astronomical Society
Clough K
(2024)
What no one has seen before: gravitational waveforms from warp drive collapse
in The Open Journal of Astrophysics
| Description | Many new discoveries about the formation and evolution of galaxies, star formation, planet formation and particle physics theory have been made possible by the award. |
| Exploitation Route | Many international collaborative projects are supported by our results |
| Sectors | Aerospace Defence and Marine Digital/Communication/Information Technologies (including Software) Education |